Radiating Cosmological Black Hole Horizons

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Ebadi, Javad | 2015

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Type of Document: M.Sc. Thesis
Language: Farsi
Document No: 47569 (04)
University: Sharif University of Technology
Department: Physics
Advisor(s): Mansouri, Reza; Taghizadeh Firouzjaee, Javad
Abstract:
One of the main subjects that has been vastly studied recently, is the final fate of Black holes with Hawking radiation. Radiation of a black hole changes the black hole, thus horizons of the black hole will also have dynamics. For a radiating black hole the inward flux of matter and the flux of radiation are two important factors for determining black hole energymomentum tensor that determine dynamics of different kinds of horizons. Quantum flux calculation needs choosing a proper quantum state as vacuum for calculating the expectation value of energy-momentum tensor. In this thesis we have attempted to write a useful reference and we hope it could help the reader to prepare for studying quantum aspects of black holes especially those questions related to backreaction of hawking radiation
Keywords:
Horizon ; Hawking Radiation ; Cosmological Black Hole ; Backreaction ; Normal Ordered Energy-Momentum-Tensor